0000000000431398

AUTHOR

Evelyne Roueff

showing 3 related works from this author

The hyperfine structure in the rotational spectrum of CF+

2012

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter lines. The origin of this double-peak profile may be kinematic or spectroscopic. Aims. We investigate the effect of hyperfine interactions due to the fluorine nucleus in CF+ on the rotational transitions. Methods. We compute the fluorine spin rotation constant of CF+ using high-level quantum chemical methods and determine the relative positions and intensities of each hyperfine component. This information is used to fit the theoretical hyperfine components to the observed CF+ line profiles, thereby employing the h…

AstrochemistryFOS: Physical sciencesContext (language use)Astrophysics010402 general chemistryRotation01 natural sciencesISM: clouds0103 physical sciencesSpin (physics)010303 astronomy & astrophysicsHyperfine structureAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsNebularadio lines: ISMastrochemistryAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesISM: molecules0104 chemical sciences[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ISM: individual objects: Horsehead nebula[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Atomic physicsBar (unit)
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Virtual atomic and molecular data centre

2010

The Virtual Atomic and Molecular Data Centre (VAMDC, http://www.vamdc.eu) is a European Union funded collaboration between groups involved in the generation, evaluation, and use of atomic and molecular data. VAMDC aims to build a secure, documented, flexible and interoperable e-science environment-based interface to existing atomic and molecular data. The project will cover establishing the core consortium, the development and deployment of the infrastructure and the development of interfaces to the existing atomic and molecular databases. It will also provide a forum for training potential users and dissemination of expertise worldwide. This review describes the scope of the VAMDC project;…

Interface (Java)InteroperabilityNanotechnology01 natural sciencesWorld Wide Web0103 physical sciencesmedia_common.cataloged_instanceEuropean union010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSpectroscopymedia_commonPhysics/dk/atira/pure/subjectarea/asjc/1600/1607/dk/atira/pure/subjectarea/asjc/3100/3108RadiationScope (project management)business.industry/dk/atira/pure/subjectarea/asjc/3100/3107Online databaseAtomic and Molecular Physics and Optics[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistryMolecular DatabasesSoftware deployment[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistryData centerbusinessJournal of Quantitative Spectroscopy and Radiative Transfer
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H-2, H-3(+) and the age of molecular clouds and prestellar cores

2012

Measuring the age of molecular clouds and prestellar cores is a difficult task that has not yet been successfully accomplished although the information is of paramount importance to help in understanding and discriminating between different formation scenarios. Most chemical clocks suffer from unknown initial conditions and are therefore difficult to use. We propose a new approach based on a subset of deuterium chemistry that takes place in the gas phase and for which initial conditions are relatively well known. It relies primarily on the conversion of H 3 + into H 2D + to initiate deuterium enrichment of the molecular gas. This conversion is controlled by the ortho/para ratio of H2 that i…

AstrochemistryAbundance (chemistry)General MathematicsGeneral Physics and AstronomySULFUR CHEMISTRYAstrophysicsINITIAL CONDITIONS01 natural sciences7. Clean energySTAR-FORMATION0103 physical sciencesGravitational collapseProtostar010306 general physics010303 astronomy & astrophysicsAMBIPOLAR DIFFUSIONCOSMIC-RAY IONIZATION[PHYS]Physics [physics]INTERSTELLAR-MEDIUMStar formationMolecular cloudTRIPLY DEUTERATED AMMONIAGeneral EngineeringORTHO-PARA TRANSITIONSInterstellar mediumDARK CLOUDSGRAVITATIONAL COLLAPSEDeuterium13. Climate action[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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